david bressoud macalester college, st. paul, mn

David Bressoud Macalester College, St. Paul, MN

NCTMAnnualMee,ngWashington,DCApril23,2009

Theseslidesareavailableatwww.macalester.edu/~bressoud/talks

“The task of the educator is to make the child’s spirit pass again where its forefathers have gone, moving rapidly through certain stages but suppressing none of them. In this regard, the history of science must be our guide.”

Henri Poincaré 1854–1912

Trigonometry

The problems:

• The emphasis on trigonometric functions as ratios of sides of various right triangles often leads students to view sine, cosine, etc. as functions of a triangle rather than an angle.

Common student and teacher difficulties with trigonometric functions have been studied by Pat Thompson and Kevin Moore at Arizona State University.

• Students are often confused about how angle measure is defined and have trouble working with radian measure of angles.

• Students have trouble making the transition to trigonometric functions as periodic functions with continuously varying input and output.

OldBabylonianEmpire,2000–1600BCE

PrincetonUniversityPress,2008

Plimpton322(ColumbiaUniversity),tableofPythagoreantriples,circa1700BCE,about9by13cm

Mathematical Association of America, 2004

SimplePythagoreantriples:

32 + 42 = 52

52 +122 = 132

82 +152 = 172

B

A

C

B

A

C

A B C

119 120 169

3367 3456 4825

4601 4800 6649

12709 13500 18541

65 72 97

319 360 481

2291 2700 3541

799 960 1249

481 600 769

4961 6480 8161

45 60 75

1679 2400 2929

161 240 289

1771 2700 3229

28 45 53

B – A

The difference between the square of side A+B and the square of side B–A is four rectangles of size AB.

A + B( )2 − B − A( )2= 4AB

A

B

If AB = ¼, then (A + B)2 and (A – B)2 differ by 1.

B + A

A = 6 5, B = 5 2465×524

=14

65−524

=119120

,

65+524

=169120

169120

⎛⎝⎜

⎞⎠⎟2

−119120

⎛⎝⎜

⎞⎠⎟2

= 1

1692 = 1192 +1202

B

A

C

A B C

119 120 169 6/5,5/24

3367 3456 4825 32/27,27/128

4601 4800 6649 75/64,16/75

12709 13500 18541 125/108,27/125

65 72 97 9/8,2/9

319 360 481 10/9,9/40

2291 2700 3541 27/25,25/108

799 960 1249 16/15,15/64

481 600 769 25/24,6/25

4961 6480 8161 81/80,20/81

45 60 75 1,1/4

1679 2400 2929 24/25,25/96

161 240 289 15/16,4/15

1771 2700 3229 25/27,27/100

28 45 53 9/10,5/18

Hipparchus of Rhodes Circa 190–120 BC

PrincetonUniversityPress,2009

earth

Winter solstice

Spring equinox

Summer solstice

Autumnal equinox

93⅝ days

earth

Winter solstice

Spring equinox

Summer solstice

Autumnal equinox

89 days

89⅞ days

92¾ days

93⅝ days

earth

center

Winter solstice

Spring equinox

Summer solstice

Autumnal equinox

89 days

92¾ days

89⅞

days

Basicproblemofastronomy:

Giventhearcofacircle,findthelengthofthechordthatsubtendsthisarc.

To measure an angle made by two line segments, draw a circle with center at their intersection.

The angle is measured by the distance along the arc of the circle from one line segment to the other.

The length of the arc can be represented by a fraction of the full circumference: 43° = 43/360 of the full circumference.

If the radius of the circle is specified, the length of the arc can also be measured in the units in which the radius is measured:

Radius = 3438, Circumference = 60×360 = 21600

Radius = 1, Circumference = 2π

92° 17'

earth center

Winter solstice

Spring equinox

Summer solstice

Autumnal equinox

87° 43'

88° 35'

91° 25'

3° 42'

52'

Find the chord lengths for 3° 42' and 52'.

The distance from the earth to the center of the sun’s orbit is found by taking half of each chord length and using the Pythagorean theorem.

Note that the chord lengths depend on the radius.

Fron,spiecefromPtolemy’sAlmagest

PeurbachandRegiomantusedi,onof1496

• Constructed table of chords in increments of ½° and provided for linear interpolation in increments of ½ minute.

• Values of chord accurate to 1 part in 603 = 216,000 (approximately 7-digit accuracy).

Ptolemy of Alexandria Circa 85–165 CE

arc = 60

chord = R

R

36°

36°

36°

x R

R + xR

=Rx

Crd 36O =5 −12

R

72°

Euclid’sElementsBook13,Proposi,on9

Thera,ooftheradiusofacircletothesideoftheregularinscribeddecahedronisequaltothegoldenra,o(“meanandextremepropor,on”).

Ry=ACR

⇒ R2 = y ⋅ AC

xBC

=yx⇒ x2 = y ⋅ BC

R2 + x2 = y2

Chord 72O =5 + 5

2R

Euclid’sElementsBook13,Proposi,on10

Thesquareofthesideoftheregularinscribeddecahedronplusthesquareoftheradiusofthecircleisequaltothesquareofthesideoftheregularinscribedpentagon.

x

y

O

A B C

D

Ptolemy’s Lemma: Given any quadrilateral inscribed in a circle, the product of the diagonals equals the sum of the products of the opposite sides.

A

B

C

D

AC ⋅ BD = AB ⋅CD + AD ⋅ BC

Ptolemy’s Lemma: Product of the diagonals equals the sum of the products of the opposite sides.

AC = 2R∠ADC = ∠ABC = 900

2R ⋅ BD = AD ⋅ BC + AB ⋅CD2R ⋅Crd α + β( )= Crdα ⋅Crd 1800 − β( )+ Crd β ⋅Crd 1800 −α( )

B

C

D

A α

β

Ptolemy’s Lemma: Product of the diagonals equals the sum of the products of the opposite sides.

AC = 2R∠ADC = ∠ABC = 900

2R ⋅ BD = AD ⋅ BC + AB ⋅CD2R ⋅Crd α + β( )= Crdα ⋅Crd 1800 − β( )+ Crd β ⋅Crd 1800 −α( )

B

C

D

A α

β

Crd 600 and Crd 720 ⇒ Crd 120

⇒ Crd 60

⇒ Crd 30

⇒ Crd 10 30 '⇒ Crd 45 '

If α < β < 900, thenCrd βCrdα

<βα

1β

Crd β <1α

Crd α

23Crd 10 30 ' < Crd 10 < 4

3Crd 45 '

⇒ Crd 10

⇒ Crd 30 '

B

C

D

A α

β

Kushan Empire

1st–3rd centuries CE

Arrived from Central Asia, a successor to the Seleucid Empire

Imported Greek astronomical texts and translated them into Sanskrit

Surya-Siddhanta

Circa 300 CE

Earliest known Indian work in trigonometry, had already made change from chords to half-chords

Ardha-jya = half bowstring

Became jya or jiva

Chord θ = Crd θ = 2 Sin θ/2 = 2R sin θ/2

R

θ θ/2

Jiya – Sanskrit Jiba (jyb) – Arabic

jyb jaib, fold or bay Sinus, fold or hollow – Latin Sine – English

ko,jya=cosine

shadow

Gnomon(sundial)

Al‐Khwarizmi,BaghdadCirca790–840

Earliestknownreferencetoshadowlengthasafunc4onofthesun’seleva,on

shadow

Gnomon(sundial)

Al‐Khwarizmi,BaghdadCirca790–840

Earliestknownreferencetoshadowlengthasafunc4onofthesun’seleva,on

shadow

Gnomon(sundial)

Al‐Khwarizmi,BaghdadCirca790–840

Earliestknownreferencetoshadowlengthasafunc4onofthesun’seleva,on

shadow

Gnomon(sundial)

Al‐Khwarizmi,BaghdadCirca790–840

Earliestknownreferencetoshadowlengthasafunc4onofthesun’seleva,on

shadow

Gnomon(sundial)

Al‐Khwarizmi,BaghdadCirca790–840

Earliestknownreferencetoshadowlengthasafunc4onofthesun’seleva,on

Abu’lWafa,Baghdad,940–998

Tangent

R

If you know the angle, θ, and the leg adjacent to that angle, the Tangent gives the length of the opposite leg.

θ

Abu’lWafa,Baghdad,940–998

Tangent

R

If you know the angle, θ, and the leg adjacent to that angle, the Tangent gives the length of the opposite leg.

The Cotangent is the Tangent of the complementary angle. If you know the angle and the length of the leg opposite that angle, the Cotangent gives the length of the adjacent leg.

R

Cotangent θ

θ

Abu’lWafa,Baghdad,940–998

Tangent

R

If you know the angle, θ, and the leg adjacent to that angle, the Tangent gives the length of the opposite leg.

The Cotangent is the Tangent of the complementary angle. If you know the angle and the length of the leg opposite that angle, the Cotangent gives the length of the adjacent leg.

R

Cotangent θ

θ Tan θR

=Sin θCos θ

Cot θR

=Cos θSin θ

Sine

Cosine

Abu’lWafa,Baghdad,940–998

Tangent Secant

If you know the angle, θ, and the leg adjacent to that angle, the Secant gives the length of the hypotenuse.

θ R

Sec θR

=R

Cos θ

Abu’lWafa,Baghdad,940–998

Tangent Cosecant

If you know the angle, θ, and the leg adjacent to that angle, the Secant gives the length of the hypotenuse.

The Cosecant is the Secant of the complementary angle. If you know the angle and the length of the leg opposite that angle, the Cosecant gives the length of the hypotenuse.

R

θ

θ

R Csc θR

=R

Sin θ

Bartholomeo Pitiscus, 1561–1613, Grunberg in Silesia

1595 published Trigonometria, coining the term “trigonometry.”

According to Victor Katz, this was the first “text explicitly involving the solving of a real plane triangle on earth.”

Leonhard Euler, 1707–1783

Standardizes the radius of the circle that defines the angle to R = 1.

If we want to apply the tools of calculus, we need to measure arc length and line length in the same units, thus the circumference of the full circle is 2π.

Euler did not use radians. For him, trigonometric functions expressed the lengths of lines in terms of the length of an arc of a circle of radius 1.

1840–1890

During this half-century, trigonometry textbooks shift from trigonometric functions as lengths of lines determined by arc lengths to ratios of sides of right triangles determined by angles.

For the first time, this necessitates a name for the angle unit used in calculus: radian. Coined independently in the 1870s by Thomas Muir and William Thomson (Lord Kelvin).

Lessons:

1.  There is a lot of good and interesting circle geometry that sits behind trigonometry.

Lessons:

2.  Ratios are intrinsically hard. It is much easier and more intuitive to think of trigonometric functions as lengths of lines.

3.  Angle as a measurement of how far something has turned is intrinsically hard. It is easier to think of trigonometric functions as functions of arc length.

4.  Rather than trying to deal with radians as the numerator in a fraction whose denominator is 2π, think of them as the distance traveled along the circumference of a circle of radius 1.

Lessons:

5.  The circle definition of the sine and cosine is much closer to the way these functions have been defined and used throughout history than is soh-cah-toa.

θ sine θ

cosine θ

Thispresenta,onisavailableatwww.macalester.edu/~bressoud/talks

R = 1